Weber / Davis Model Revisited - Standing Magnetohydrodynamic Shocks in Accretion and Winds

Details Weber / Davis Model Revisited - Standing Magnetohydrodynamic Shocks in Accretion and Winds Weber / Davis Model Revisited - Standing Magnetohydrodynamic Shocks in Accretion and Winds

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.246..134c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 246, NO. 1/SEP1, P. 134, 1990

Mathematics

Logic

8

Scientific paper

All the topologically distinct solutions of the Weber-Davis model for
magnetized astrophysical flows are presented. This paper concentrates on
the solutions which allow self-consistent magnetohydrodynamic shocks in
the conical accretion and' wind flows around a compact magnetic star.
Examples of such shocks are provided.

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